Inflation on Fractional Branes: D--Brane Inflation as D--Term Inflation
arXiv:hep-th/0312042 · doi:10.1088/1126-6708/2004/07/080
Abstract
We describe a D--brane inflation model which consists of two fractional D3 branes separated on a transverse . Inflation arises due to the resolved orbifold singularity of which corresponds to an anomalous D--term on the brane. We show that D--brane inflation in the bulk corresponds to D--term inflation on the brane. The inflaton and the trigger field parametrize the interbrane distances on an respectively. After inflation the branes reach a supersymmetric configuration in which they are at the origin of but separated along the directions.
15 pages in phyzzx.tex; minor corrections including all factors of 2π; v3: more minor corrections
References in corpus (9)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
- Non-commutative superspace from string theory
- Effective Field Theories and Inflation
- Four Lectures On The Gauge/Gravity Correspondence
- Fermions scattering in a three dimensional extreme black hole background
- D-brane Dynamics and Creations of Open and Closed Strings after Recommbination
- Brane Inflation from Rotation of D4 Brane
Cited by in corpus (7)
- Encyclopaedia Inflationaris
- Particle physics models of inflation and curvaton scenarios
- Overproduction of cosmic superstrings
- Slow Roll in Brane Inflation
- Formation of monopoles and domain walls after brane inflation
- Power of Black Hole Physics: Seeing through the Vacuum Landscape
- Defect Formation with Bulk Fields